新魁北克陨石坑的鉴定争议和岩石学影响

U. Marvin, D. Kring
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引用次数: 17

摘要

1949年,根据一张航拍照片,新魁北克陨石坑在加拿大地盾的前寒武纪片麻岩中呈现出独特的圆形和凸起的边缘,有人提出它是陨石形成的。当时,只有那些与陨石有关的少数陨石坑被普遍认为是撞击的起源。当最早的实地考察未能找到陨石或撞击产物时,两位著名的陨石学家弗雷德里克·c·伦纳德和林肯·拉帕兹把“丘布”陨石坑作为一个明目张神的例子,证明在没有有效证据的情况下就提出了陨石起源的主张。他们还把阿散蒂(现在的加纳)的博萨姆特维湖陨石坑列为类似陨石坑的特征之一,显然不是陨石形成的,被误认为是陨石坑。关于这两个陨石坑起源的争论持续了几十年。在本文的第一部分中,我们追溯了导致目前接受新魁北克作为真实撞击坑的调查。我们注意到,由于尚不完全清楚的原因,新魁北克陨石坑的陨石起源在更早的时候获得了比博苏姆特维湖陨石坑更广泛的接受,后者的岩石学和化学证据更为丰富和令人信服。在第二部分中,我们描述了来自新魁北克陨石坑的两个撞击熔体样品的岩石学,并提供了影响辅助矿物磷灰石、榍石、磁铁矿和锆石的冲击变质程度的新证据。尤其是锆石,呈现出从无蚀变迹象的自面体颗粒到分解成坏辉石+二氧化硅颗粒的变化范围。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Authentication controversies and impactite petrography of the New Quebec Crater
— A meteoritic origin was proposed for the New Quebec Crater in 1949 on the basis of an aerial photograph showing its unique circularity and raised rim amid Precambrian gneisses of the Canadian Shield. At that time, only those few craters associated with meteorites were generally accepted as of impact origin. When the earliest field expeditions failed to find meteorites or impact products, two leading meteoriticists, Frederick C. Leonard and Lincoln LaPaz, cited the “Chubb” Crater as a flagrant example for which claims of meteoritic origin were advanced without valid proof. They also listed the Lake Bosumtwi Crater in Ashanti (now Ghana) among crater-like features, clearly of non-meteoritic origin, misidentified as meteorite craters. Controversy over the origin these two craters continued for decades. In Part I of this paper, we trace the investigations that led to the current acceptance of New Quebec as an authentic impact crater. We note that, for reasons that are not entirely clear, a meteoritic origin for the New Quebec Crater achieved wider acceptance at an earlier date than for the Lake Bosumtwi Crater, where petrographic and chemical evidence is more abundant and compelling. In Part II, we describe the petrography of two impact melt samples from the New Quebec Crater and present new evidence on the degrees of shock metamorphism affecting the accessory minerals: apatite, sphene, magnetite and zircon. Zircon, in particular, shows a range from euhedral grains with no signs of alteration to those decomposed to baddeleyite plus silica.
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